The performance of GaAs/AlGaAs multiple quantum well infrared detector
s is studied theoretically and experimentally, with special emphasis o
n 8-12 mu m thermal imaging applications. The dependence of detector p
erformance on various factors like light coupling configurations (one
and two dimensional reflection gratings or 45 degrees polished edge),
detector temperature, response wavelength and quantum well doping dens
ity is dealt with. An absorption quantum efficiency of 87% is demonstr
ated using a crossed grating and a waveguide (CGW). It is also found t
hat an optimised 341 mu m x 34 mu m detector (a detector size suitable
for large staring arrays, i.e. 256 x 256 or larger) with 9.0 mu m cut
-off wavelength, f# = 2 optics and 70% optical transmission reaches ba
ckground limited operation at 74K detector temperature. The potential
of making highly uniform staring arrays utilising the mature GaAs mate
rial and processing technology is demonstrated by uniformity measureme
nts of detector dark current. The experiments show that a metalorganic
vapour phase epitaxy (MOVPE) grown structure can have a dark current
standard deviation to mean value ratio over a 10mm long linear detecto
r array of less than 2%. The staring array performance in terms of noi
se equivalent temperature difference (temporal NETD) is calculated to
NETD < 20mK at 77K detector temperature and NETD < 10 mK at 70K detect
or temperature.